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Asymmetric Neutrino Emission from Magnetized Proto-Neutron Star Matter including Hyperons in Relativistic Mean Field Theory

We calculate asymmetric neutrino absorption and scattering cross sections on hot and dense magnetized neutron-star matter including hyperons in fully relativistic mean field theory. The absorption/scattering cross sections are suppressed/enhanced incoherently in the direction of the magnetic fielld, B. The asymmetry is 2-4% at the matter density ρ_0 < ρ_B < 3ρ_0 and temperature T < 40 MeV for B=2 X 10^{17} G. This asymmetry is comparable to the effects owing to parity violation or asymmetric magnetic field topology proposed for the origin of pulsar kicks.

preprint2013arXivOpen access
Tomoyuki MaruyamaToshitaka KajinoNobutoshi YasutakeMyung-Ki CheounChung-Yeol Ryu
nucl-thastro-ph.SR
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Tomoyuki MaruyamaToshitaka KajinoNobutoshi YasutakeMyung-Ki CheounChung-Yeol Ryu

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